The magnetorotational instability prefers three dimensions

DOI10.1098/rspa.2019.0622zbMath1472.85003arXiv1912.00972OpenAlexW2999622274WikidataQ89819578 ScholiaQ89819578MaRDI QIDQ5160860

Daniel Lecoanet, Keaton J. Burns, Andrew Swan, Jeffrey S. Oishi, Benjamin P. Brown, Geoffrey M. Vasil, Morgan Baxter

Publication date: 29 October 2021

Published in: Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1912.00972

zbMATH Keywords

starsstabilityastrophysicsmagnetohydrodynamicsplasma physicsfluid mechanics

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Magnetorotational instability: recent developments
• Magnetorotational instability of dissipative Couette flow
• On the magnetorotational instability and elastic buckling

This page was built for publication: The magnetorotational instability prefers three dimensions